and Cosmology

Subject Index
455
Doppler effect 38
Doppler favoritism 211
Doppler shift 10
Doppler width 11, 196
downsizing 401
drop-out technique see Lyman-break
technique
dust 41, 208
– extinction and reddening 41, 328,
373
– gray dust 329
– infrared emission 51, 90, 102, 196,
208, 369, 374
– warm dust 196, 208, 371, 374
dwarf galaxies see galaxies
dynamical friction 235, 238, 397, 400
dynamical instability of N-body
systems 85
dynamical pressure 47
E
early-type galaxies 88
Eddington accretion rate 194
Eddington efficiency 205, 206
Eddington luminosity 193–194, 205,
207, 371, 402
effective radius R e 55, 90, 107
effective temperature 425, 426
Effelsberg radio telescope 19
Einstein observatory 31, 255
Einstein radius θ E see gravitational
lenses
Einstein–de Sitter model
see Universe
elliptical galaxies see galaxies
emission coefficient 418
energy density of a radiation field 417
equation of radiative transfer 40, 417
equivalent width 181, 332
expansion rate see cosmology
Extended Medium Sensitivity Survey
(EMSS) 255
extinction 40, 328
– extinction and reddening 40, 328
– extinction coefficient 41, 422
extremely red object (ERO) 371–374,
391, 394
F
Fanaroff–Riley classification 178,
184
Faraday rotation 52, 212
feedback 360, 396
fermions 160
Fingers of God 316, 317
fireball model see gamma-ray bursts
flatfield 236
flatness problem 172, 174, 307
flux 417
free–free radiation 242
Freeman law 99, 105
free-steaming 286
Friedmann equations 149, 289
Friedmann–Lemaître model 15, 149
fundamental plane 107–108, 319,
392
FUSE 30, 335
G
GAIA 38, 411
Galactic center 6, 77–84
– black hole 80–85
– distance 45, 56
– flares 82
Galactic coordinates 35–36
Galactic latitude 35
Galactic longitude 35
Galactic poles 35
galaxies 7–8, 87–140
– bimodal color distribution 119
– brightness profile 90–92, 98
– cD galaxies 90, 92, 230, 237, 249,
264
– chemical evolution 138–140
– color–color diagram 357
– dwarf galaxies 90, 224
– E+A galaxies 241
– early-type galaxies 8
– elliptical galaxies 88, 90–98
blue compact dwarfs (BCD’s) 90
classification 88, 90
composition 92–93
counter-rotating disks 96
dark matter 101
dwarf ellipticals (dE’s) 90
dwarf spheroidals (dSph’s) 90
dynamics 93–95
formation 392–395
indicators for complex evolution
95–98, 393
mass-to-light ratio 96
stellar orbits 94
– halos 100
– Hubble sequence 88
– IRAS galaxies 368, 370
– irregular galaxies 88, 224
– late-type galaxies 8
– low surface brightness galaxies
(LSBs) 99, 301
– luminosity function 117–119
– Lyman-break galaxies 367, 391
– morphology–density relation 360
– post-starburst galaxies 241
– S0 galaxies 88, 393
– satellite galaxies 101, 224, 304, 360
– scaling relations 104–109, 116, 319
– SCUBA galaxies 374–377
– spheroidal component 111, 113
– spiral galaxies 88, 98–104
bars 88
bulge 98, 102, 397
corona 103
dark matter 100
early-type spirals 98
normal and barred 88
rotation curve 8, 100–102, 104
spiral structure 103
stellar halo 100
stellar populations 102
thick disk 100
– starburst galaxies 11, 89, 203, 358,
369–371
– substructure 302–306, 396
– ULIRG (ultra-luminous infrared
galaxy) 24, 90, 208, 370
galaxy evolution 17, 390–402
galaxy groups 223, 228, 237–238
– compact groups 237, 238
– diffuse optical light 238
GALEX 31, 361
gamma-ray bursts
– afterglows 404
– fireball model 404
– hypernovae 405
– short- and long-duration bursts 404
G-dwarf problem 140
globular clusters 55, 102
GOODS project 366